2019
DOI: 10.1216/jie-2019-31-4-535
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A new class of Volterra-type integral equations from relativistic quantum physics

Abstract: Here we study a new kind of linear integral equations for a relativistic quantummechanical two-particle wave function ψ(x 1 , x 2 ), where x 1 , x 2 are spacetime points. In the case of retarded interaction, these integral equations are of Volterra-type in the in the time variables, i.e., they involve a time integration from 0 to t i = x 0 i , i = 1, 2. They are interesting not only in view of their applications in physics, but also because of the following mathematical features: (a) time and space variables a… Show more

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Cited by 19 publications
(32 citation statements)
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“…In Sec. 4.1, we show that the theorems in [18] carry over to the case of flat FLRW universes. The main result are rigorous existence and uniqueness theorems for a class of integral equations with sufficiently regular interaction kernels for d = 1, 2, 3 dimensions (Thms.…”
Section: Introductionmentioning
confidence: 64%
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“…In Sec. 4.1, we show that the theorems in [18] carry over to the case of flat FLRW universes. The main result are rigorous existence and uniqueness theorems for a class of integral equations with sufficiently regular interaction kernels for d = 1, 2, 3 dimensions (Thms.…”
Section: Introductionmentioning
confidence: 64%
“…In this section, we formulate the integral equation (2) on a (1+d)-dimensional Minkowski half-space for d = 1, 2, 3. After that, we state the existence and uniqueness results of the previous paper [18]. We shall give the full details, as they are necessary later in the paper.…”
Section: Previous Results For a Minkowski Half-spacementioning
confidence: 97%
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“…In recent years, there has been a renewed interest in constructing mathematically rigoros multi-time models, see [5] for an overview. Some of the current efforts to understand Dirac's multi-time models focus on the well-posedness of the corresponding initial value problems [6,7,8,9,10], other works also ask the question how the multi-time formalism could be exploited to avoid the infamous ultraviolet divergence of relativistic QFT and how a varying number of particles by means of creation and annihilation processes can be addressed [11,12,13]. Beside being candidate models for fundamental formulations of relativistic wave mechanics, a better mathematical understanding of such multi-time evolutions may also be beneficial regarding more technical discussions, such as the control of scattering estimates on vacuum expectation values of products of interacting field operators; see e.g.…”
Section: The Need For Multi-time Modelsmentioning
confidence: 99%